QRZ! Ham Radio 3/QRZ Ham Radio Callsign Database - Volume 3.iso/digests/infoham/931523.txt

Internet Message Format | 1994-06-04 | 25KB

Date: Thu, 30 Dec 93 04:30:05 PST
From: Info-Hams Mailing List and Newsgroup <[e-mail]>
Errors-To: [e-mail]
Reply-To: [e-mail]
Precedence: Bulk
Subject: Info-Hams Digest V93 #1523
To: Info-Hams


Info-Hams Digest            Thu, 30 Dec 93       Volume 93 : Issue 1523

Today's Topics:
               Balloon to launch carrying amateur radio
                      Cell phones & hearing aids
                            childish stuff
                             cw waivers
     Daily Summary of Solar Geophysical Activity for 29 December
                  Free Tailgate Party - Orlando, FL
                         RACES Bulletin #306
                         RFI into telephones
                                TM732A

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We trust that readers are intelligent enough to realize that all text
herein consists of personal comments and does not represent the official
policies or positions of any party.  Your mileage may vary.  So there.
----------------------------------------------------------------------

Date: Thu, 30 Dec 1993 07:45:11 GMT
From: swrinde!sgiblab!a2i![e-mail]
Subject: Balloon to launch carrying amateur radio
To: [e-mail]

                  Superpressure Balloon Launch

A cooperative group from Utah State University, Logan, Utah,
members of the amateur radio community, and Winzen International
plan on launching SuperBall 1-94 at approximately 10:00 A.M. MST
(17:00 UTC) on January 5, 1994 from the Logan Municipal Airport.
The nylon superpressure balloon for this flight is 76 feet in
diameter.  It was manufactured and donated by Winzen
International of San Antonio, Texas.  The expected daytime float
altitude of this helium filled balloon will be 120,000 ft (36,660
meters), some loss of altitude is expected at night.
Theoretically the technology is capable of maintaining a payload
at altitude for long periods of time, potentially years.

The initial track of SuperBall will depend on upper air conditions
at the time of launch, but is expected to be in the semicircle east
from Utah. Possible scenarios might then take it over the Atlantic
Ocean or into the polar regions within a few days.

The payload will be limited to a gross weight of 4 kilograms, or
8.8 pounds.  It will consist of the following subsystems:

1. An instrument package containing a five channel Magellan GPS
receiver, an external air temperature sensor, an internal payload
temperature sensor, a battery voltage sensor, and a differential
pressure gauge.

2.  A 1/2-watt VHF MCW beacon operating on 145.871 MHz with the
callsign N7YTK. Every minute it will transmit data from
instruments listed above. (This transmitter will also operate
through the Russian RS-10 amateur satellite, which has a downlink
frequency 29.371 MHz, plus or minus Doppler.)

3.  A one-watt CW 15-meter beacon operating on 21.229 MHz with a
call sign of WB8ELK.  Every five minutes it will transmit data
identical to that sent on the 145.871 MHz beacon.  (This signal will
also be relayed through the Russian RS-12 amateur satellite, which
has a downlink frequency of 29.429 MHz, plus or minus Doppler.)

4.  An ATV system consisting of a black-and-white CCD camera and
associated one-watt transmitter operating on 434.00 MHz in
continuous bursts on command.

5.  A cutdown package containing a VHF command receiver, DTMF
decoder and barometric switch, and

6.  Several Lithium battery packs.

Depending on weight availability, two additional beacons are
possible:

7.  A one-watt VHF AFSK beacon transmitting ASCII data at 1200 baud
on 145.968 MHz every two minutes in alteration with the beacon in
(2) above, with the call sign of WB8ELK (also operating through the
Japanese FO-20 satellite, which has a downlink frequency of 435.832
MHz), and

8.  A 60-milliwatt 10-meter CW beacon operating on 28.322 MHz every
minute, with a call sign of WB8ELK, transmitting pressure altitude,
internal temperature, external temperature and battery voltage. Item
(8) will contain either a 9-volt lithium pack that should last a
month, or a 9-volt, 150 ma solar panel, lasting indefinitely.

The purpose of the SuperBall 1-94 mission is to certify this
superpressure balloon technology for long-duration flight and to
test our ability to control and receive data from a high-altitude
research balloon for an extended period of time.

Our first plateau of success will be achieved if we operate
through a complete sunset/sunrise cycle at a constant pressure
altitude.  Our second plateau will be a flight lasting a week.
Our third plateau will be a complete circumnavigation of the
globe.  Anything after that is gravy.

The float path of the balloon is very difficult to predict since
the polar breakout usually occurs is this time of year frequently
resulting in strong north-south currents.

Observers from the Jet Propulsion Laboratory, Martin Marietta and
Utah State University's Space Dynamics Laboratory will be present
at the launch.  These people are potential users of the
superpressure balloon for a Martian mission.

An HF net will be conducted by John Luker, WB7QBC, (Internet
[e-mail]) on the day of the launch and
subsequent days on 7230 KHz +-QRM.  This net will alert
interested hams downrange of the balloon's path, and coordinate
the collection of telemetry.  The Utah Balloon Team would
appreciate the forwarding of any telemetry copied to John's
address along with pertinent information, including the receiving
station's location, UTC date and time, signal report, and
receiving equipment.  Video tapes of any received ATV
transmissions from the balloon would also be appreciated.  At
this point we only anticipate turning the camera on during the
first two days.

Questions can be directed to Bruce Bergen, KI7OM, through
Internet at [e-mail]


--
Gordon R. Smith, K7HFV        [e-mail]
Salt Lake City, Utah

------------------------------

Date: Thu, 30 Dec 1993 07:47:57 GMT
From: netcomsv!netcom.com![e-mail]
Subject: Cell phones & hearing aids
To: [e-mail]

Fellow hams,

Could one of you please explain the alleged interaction (interference)
between cellular telephones and FM hearing aids for hard-of-hearing
people?

I'll summarize and post back here and the deaf mailing list.

Thx.  :-)  M

-----------------------------------------------------------------------

Esther A. Paris ([e-mail]) wrote:
: Can someone kindly explain to me why/how the cell phones are
: causing problems for FM users?

: My husband (a follower of telecom news) couldn't explain to me
: why cell phones interfere with the FM systems for deaf/HoH people.

: He also had this to say:

: (begin fragment from note Esther's husband sent)
: *I don't know what cell phones have to do with FM hearing aid
: *systems.  I'll be surprised to hear that they use the same
: *frequencies.
: *
: *Even if there is some kind of interference problem, the situation
: *should start improving over the next several years.  The new
: *system for cellular telephony will probably be CDMA (Code Division
: *Multiple Access) and it uses a spread-spectrum communications
: *system.  Spread-spectrum should not interfere with any FM based
: *system.  Of course, it'll take a while before the old system
: *is completely phased out....
: (end fragment from note Esther's husband sent)

: Please let me know!  Curious to the extreme, Esther Paris
--

------------------------+------------------------+---------------------------
Michael Sattler, KE6DZF |  All that is required  |  Encrypt now; ask me how.
Digital Jungle Software |  for evil to triumph   |  Finger for PGP key.
  [e-mail]   | is for {wo}men of good |  GCSy+n+f+g+t+d--p--c++u+
    +1.415.621.2903     |   will to do nothing.  |  e+m++s++/rhw!l

------------------------------

Date: 30 Dec 1993 04:30:08 GMT
From: swrinde!cs.utexas.edu!geraldo.cc.utexas.edu!astro.as.utexas.edu![e-mail]
Subject: childish stuff
To: [e-mail]

[e-mail] (Gary Coffman) drones on and on and on:

(someone else said)
>>Oh yes, you do understand that DXing and contesting are two very
>>different things, right?  Your original post seemed somewhat confused
>>about that.

Gary says:
>They're both compulsive activities done for score. Contests are usually
>shorter and with different ways of counting points. DXing is postal card
>collecting with a masochistic twist, and a maximum score of 319. It's an
>obsessive compulsive behavior.

Gary, old chap - please make a 1994 resolution to grow up.  You have
made your points that (a) you don't like CW, and (b) you don't like
the ARRL.  Not once but several hundred times.  I'm sure I don't like
some of the things that you like doing, but I don't keep posting stuff
here saying that they are worthless pursuits.  In areas where you seem
to know what you are talking about, I will respect your knowledge and
advice.  But as another poster said, please stick to the things that
you do understand.

I have no idea where your number 319 comes from - my "score" is more
than that, and I certainly haven't worked every country on the current
DXCC list.

Derek Wills (AA5BT, G3NMX)
Department of Astronomy, University of Texas,
Austin TX 78712.  (512-471-1392)
[e-mail]

------------------------------

Date: Thu, 30 Dec 93 07:18:30 GMT
From: netcomsv!netcomsv!bongo!skyld![e-mail]
Subject: cw waivers
To: [e-mail]

In article <[e-mail]> [e-mail] writes:

  > Actually since W is not needed and it not any kind fo a reliable indicator
  > of technical or operating comptetance I say hurray. CW as a requirement
  > should be eliminated. It is an outmoded method of communication and is
  > wrothwhile only as a fun test of a particular skill. TI has no relavanve
  > whatsoever to competance in any other phase of the hobby. I say that it
  > is jsut taking up too much of the ham bands. MUCH more space should be
  > allocated to the efficient digital modes such  as pactor and more communi-
  > cation could be carried out. Even hf packet would be much better if all
  > were not forced to operate on a very narrow range of frequencies. Come
  > out of the dark ages and into the light.

  Lucky for you that typing skills aren't what is required for a license....



 Amateur: WA6FWI@WA6FWI.#SOCA.CA.USA.NA  |  "It is difficult to imagine our
Internet: [e-mail]          |  universe run by a single omni-
 US Mail: PO Box 4425 Carson, CA 90749   |  potent god. I see it more as a
   Phone: [phone]               |  badly run corporation."

------------------------------

Date: Wed, 29 Dec 1993 22:29:03 MST
From: galaxy.ucr.edu!library.ucla.edu!europa.eng.gtefsd.com!howland.reston.ans.net!math.ohio-state.edu!cyber2.cyberstore.ca!nntp.cs.ubc.ca!alberta!nebulus!ve6mgs![e-mail]
Subject: Daily Summary of Solar Geophysical Activity for 29 December
To: [e-mail]

                /\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\

                 DAILY SUMMARY OF SOLAR GEOPHYSICAL ACTIVITY

                                29 DECEMBER, 1993

                /\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\/\

                  (Based In-Part On SESC Observational Data)


SOLAR AND GEOPHYSICAL ACTIVITY INDICES FOR 29 DECEMBER, 1993
------------------------------------------------------------

NOTE: The Aleutian high has intensified over the last several days.  New
      stratospheric warming is also being observed over eastern Siberia.

!!BEGIN!! (1.0) S.T.D. Solar Geophysical Data Broadcast for DAY 363, 12/29/93
10.7 FLUX=128.7  90-AVG=099        SSN=112      BKI=0110 0000  BAI=000
BGND-XRAY=B6.7     FLU1=6.6E+05  FLU10=1.1E+04  PKI=1110 1111  PAI=003
  BOU-DEV=004,005,006,004,004,004,003,002   DEV-AVG=004 NT     SWF=00:000
 XRAY-MAX= C9.4   @ 1549UT    XRAY-MIN= B5.9   @ 1926UT   XRAY-AVG= B9.7
NEUTN-MAX= +002%  @ 0610UT   NEUTN-MIN= -002%  @ 1000UT  NEUTN-AVG= +0.0%
  PCA-MAX= +0.1DB @ 1935UT     PCA-MIN= -0.4DB @ 1840UT    PCA-AVG= -0.0DB
BOUTF-MAX=55352NT @ 1426UT   BOUTF-MIN=55333NT @ 1846UT  BOUTF-AVG=55346NT
GOES7-MAX=P:+000NT@ 0000UT   GOES7-MIN=N:+000NT@ 0000UT  G7-AVG=+069,+000,+000
GOES6-MAX=P:+124NT@ 1704UT   GOES6-MIN=N:-054NT@ 0938UT  G6-AVG=+093,+029,-037
 FLUXFCST=STD:135,130,125;SESC:135,130,125 BAI/PAI-FCST=025,030,020/025,035,020
    KFCST=3334 5444 4445 5544  27DAY-AP=039,037   27DAY-KP=4555 4455 6565 4332
 WARNINGS=*SWF;*MAJFLR
   ALERTS=
!!END-DATA!!

NOTE: The Effective Sunspot Number for 28 DEC 93 was  56.0.
      The Full Kp Indices for 28 DEC 93 are: 0o 1- 0+ 0o   1- 1o 2o 2-


SYNOPSIS OF ACTIVITY
--------------------

             Solar activity was low. Region 7640 (N09W52) produced
       only three C-class flares this period, the largest being a
       C9/SF flare at 29/1549UT. This region retained its magnetic
       complexity and has begun to show penumbral growth again. New
       Region 7646 (S10E69), numbered early in the period, produced a
       single C-class flare. Region 7645 (N11E67) was also numbered
       this period.

            Solar activity forecast:  solar activity is expected to be
       low to moderate. Region 7640 still has a fair chance of an
       occasional M-class flare and an outside chance of an isolated
       X-class flare. Regions 7645 and 7646 both have a chance of an
       isolated M-class flare.

            The geomagnetic field has been at quiet levels for
       the past 24 hours.

            Geophysical activity forecast:  the geomagnetic field is
       expected to be quiet to active owing to a favorably positioned
       coronal hole.

            Event probabilities 30 dec-01 jan

                             Class M    60/60/60
                             Class X    05/05/05
                             Proton     05/05/05
                             PCAF       Green

            Geomagnetic activity probabilities 30 dec-01 jan

                        A.  Middle Latitudes
                        Active                25/30/30
                        Minor Storm           20/30/30
                        Major-Severe Storm    05/10/10

                        B.  High Latitudes
                        Active                30/30/30
                        Minor Storm           25/30/30
                        Major-Severe Storm    15/15/15

            HF propagation conditions were normal over all regions.
       Conditions are expected to become degraded on 30 or 31 December
       due to coronal hole effects.  Poor to very poor propagation
       should dominate over the high and polar latitude paths if the
       disturbance materializes.  Middle latitudes should see mostly
       good to occasionally fair propagation, with poorest propagation
       occuring over all regions during the night sector periods.


COPIES OF JOINT USAF/NOAA SESC SOLAR GEOPHYSICAL REPORTS
========================================================

REGIONS WITH SUNSPOTS. LOCATIONS VALID AT 29/2400Z DECEMBER
-----------------------------------------------------------
NMBR LOCATION  LO  AREA  Z   LL   NN MAG TYPE
7640  N09W52  205  0740 FKI  17  036 BETA-GAMMA-DELTA
7641  N05W47  200  0090 HSX  02  001 ALPHA
7644  N10W39  192  0040 CRO  06  008 BETA
7645  N11E67  086  0430 DAO  08  011 BETA
7646  S10E69  084  0170 DAO  08  006 BETA
7643  S18E03  150                    PLAGE
REGIONS DUE TO RETURN 30 DECEMBER TO 01 JANUARY
NMBR LAT    LO
NONE


LISTING OF SOLAR ENERGETIC EVENTS FOR 29 DECEMBER, 1993
-------------------------------------------------------
BEGIN  MAX  END  RGN   LOC   XRAY  OP 245MHZ 10CM   SWEEP
NONE



POSSIBLE CORONAL MASS EJECTION EVENTS FOR 29 DECEMBER, 1993
-----------------------------------------------------------
 BEGIN        MAX      END     LOCATION   TYPE   SIZE  DUR  II IV
29/A0949             B2320       S05E31   DSF


INFERRED CORONAL HOLES. LOCATIONS VALID AT 29/2400Z
---------------------------------------------------
               ISOLATED HOLES AND POLAR EXTENSIONS
      EAST   SOUTH  WEST   NORTH  CAR  TYPE  POL  AREA   OBSN
55   N59E38 S13W24 N30W45 N59W22  170  EXT   POS   058 10830A


SUMMARY OF FLARE EVENTS FOR THE PREVIOUS UTC DAY
------------------------------------------------

 Date   Begin  Max   End  Xray  Op Region  Locn    2695 MHz  8800 MHz  15.4 GHz
------  ----  ----  ----  ----  -- ------ ------  --------- --------- ---------
28 Dec: 0022  0027  0031  C1.7
        0152  0157  0207        SF  7640  N07W25
        0245  0254  0306  C8.4  SF  7640  N09W24
        0240  0243  0258        SF  7644  N10W15
        0530  0534  0537  C2.6
        0648  0652  0656  C3.0  SF  7644  N11W16
        0756  0803  0816        SF  7640  N05W33
        0833  0836  0846        SF  7640  N04W35
        0857  0904  0910  C2.7  SF  7640  N06W34        29        21
        1013  1015  1026        SF  7644  N11W18
        1059  1104  1108  C2.1
        1205  1210  1214  C4.6                         130        25
        1310  1315  1329  C1.7
        1530  1534  1538        SF  7640  N08W36
        1609  1613  1616  C2.6  SF  7644  N13W19
        2002  2005  2018        SF  7640  N08W35
        2138  2143  2150  C1.1
        2153  2157  2206        SF  7640  N07W39
        2220  2221  2224        SF  7640  N06W42
        2244  2307  2322  C5.0


REGION FLARE STATISTICS FOR THE PREVIOUS UTC DAY
------------------------------------------------

                C   M   X     S   1   2   3   4   Total   (%)
               --  --  --    --  --  --  --  --    ---  ------
  Region 7640:  2   1   0     9   1   0   0   0    010  (47.6)
  Region 7644:  2   0   0     4   0   0   0   0    004  (19.0)
Uncorrellated: 7   0   0     0   0   0   0   0    007  (33.3)

 Total Events: 021 optical and x-ray.


EVENTS WITH SWEEPS AND/OR OPTICAL PHENOMENA FOR THE LAST UTC DAY
----------------------------------------------------------------

 Date   Begin  Max   End  Xray  Op Region  Locn    Sweeps/Optical Observations
------  ----  ----  ----  ----  -- ------ ------   ---------------------------
28 Dec: 2244  2307  2322  C5.0                     III

NOTES:
     All times are in Universal Time (UT).  Characters preceding begin, max,
     and end times are defined as:  B = Before,  U = Uncertain,  A = After.
     All times associated with x-ray flares (ex. flares which produce
     associated x-ray bursts) refer to the begin, max, and end times of the
     x-rays.  Flares which are not associated with x-ray signatures use the
     optical observations to determine the begin, max, and end times.

     Acronyms used to identify sweeps and optical phenomena include:

          II        = Type II Sweep Frequency Event
          III       = Type III Sweep
          IV        = Type IV Sweep
          V         = Type V Sweep
          Continuum = Continuum Radio Event
          Loop      = Loop Prominence System,
          Spray     = Limb Spray,
          Surge     = Bright Limb Surge,
          EPL       = Eruptive Prominence on the Limb.


**  End of Daily Report  **

------------------------------

Date: Wed, 29 Dec 1993 14:13:06 EDT
From: usc!howland.reston.ans.net!usenet.ins.cwru.edu!news.ecn.bgu.edu!psuvax1!psuvm!ucf1vm![e-mail]
Subject: Free Tailgate Party - Orlando, FL
To: [e-mail]

   The University of Central Florida will hold a free Tailgate Party
at the main campus of UCF near Orlando, FL on January 8, 1994 from
7:00 AM until NOON.  This event is sponsored by the UCF-ARC and has free
admission as well as free tailgating.  There will be no food or drinks
available so you will have to bring your own.
   We usually have about 70 - 100 tailgaters and several hundred hams
show up for this event, so it is a good palce to get together and swap
ham stories and ham gear.  Everyone is welcome.

   I hope to see many hams there.

                                 Sincerely,
                                 John - kr4ah.

DISCLAIMER - I am not responsible for the actions of any Alpha-Hotels
             other than myself.

------------------------------

Date: 30 Dec 93 04:19:37 GMT
From: [e-mail]
Subject: RACES Bulletin #306
To: [e-mail]

Bid: $RACESBUL.306

TO:    ALL ES, CD, AND PUBLIC SAFETY DIRECTORS VIA AMATEUR RADIO
INFO:  ALL RACES OPERATORS IN CALIFORNIA
INFO:  ALL AMATEUR RADIO OPERATORS
FROM:  CA STATE OFFICE OF EMERGENCY SERVICES   ([e-mail])
          2800 MEADOWVIEW RD., SACRAMENTO, CA 95832 916-262-1600
          LANDLINE BBS OPEN TO ALL 916-262-1657
RACESBUL.306                 RELEASE DATE:  December  27th, 1993
SUBJECT:  MGT  -  Observations  -  Part 2/3
     I don't wish to imply that our RACES and other volunteer
government communications programs were not free of this in California
before the State Legislature undertook to turn this around. Following
authorizing legislation the State Office of Emergency Services
initiated a fulltime volunteer communications coordination effort in
1985 that has paid dividends ever since.
     Our State cannot tell the counties what do any more than counties
can dictate to cities. Therefore it is important for state government
to maintain a fulltime leadership role to maximize the positive and
productive use of unpaid communications professionals in government
service. It is such commitment to a program that makes ACS, RACES or
similar communications reserve a success --- not disasters.
     On the same multi-state RACES program trip I had the opportunity
to talk with and meet several county radio officers. Almost all of
them receive the RACES Bulletins by packet radio, by mail, and/or by
computer disk. They had established successful programs under their
emergency management officials. Some called it RACES. Others called it
the Auxiliary Communications Service, the Sheriff's Communications
Reserve and by other names. All agreed that their programs either
always or finally succeeded for several reasons, as given in the next
Bulletin.

HAPPY NEW YEAR TO ALL!

-----------------
RACES Bulletins are archived on the Internet at ucsd.edu in hamradio/races
and can be retrieved using FTP.

------------------------------

Date: Wed, 29 Dec 93 23:24:03 MST
From: swrinde!gatech!asuvax!ennews!stat![e-mail]
Subject: RFI into telephones
To: [e-mail]

[e-mail] (David Adams) writes:

> |places from my telephone wiring.  This causes RFI into my telephone
> |system.
> |
> |Any suggestions on minimizing this?

> Move the phone?
>
> Ok, Move the antenna?

Not possible in either situation ... I am one of those unfortunate that
live in an area with CC&R.  Luckily, when my house was being built, the
electrician for the builder and I installed my G5RV antenna in the attic
and crawl space.  The phone company laid its cables later ... No way to
move either.

david

---
Editor, HICNet Medical Newsletter
Internet: [e-mail]                 FAX: [phone]
Bitnet  : ATW1H@ASUACAD

------------------------------

Date: Thu, 30 Dec 1993 02:53:25 GMT
From: library.ucla.edu!agate!iat.holonet.net!takeone![e-mail]
Subject: TM732A
To: [e-mail]

Hi Corey,
        I saw your message about the 732. And i was just wondering
if you had any trouble with it. Ex the power output, its receving
sensibility or anything like that.
       Cause my father had alot of trouble with his, while my 732
works fine.
      Anyways if you do get an answer on how to make a packet cable
or buying on can you let me know. My father wants to do packet.
73's
sylvain

------------------------------

End of Info-Hams Digest V93 #1523
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